Coarse-graining support: Support.Deterministic.WeakFluxRHS.CorrectorEnergyPoincare #
Imported from the Apache-2.0 CoarseGraining development at commit
c7ddd76c08ade64fed1b8d2ca51be14dfee8deb4.
Corrector energy from the RHS Poincare estimate #
This leaf closes the manuscript Step 3.2.3 estimate for the local mean-zero
Neumann corrector: the centered energy identity gives E <= C W G, the
RHS Poincare estimate bounds W, and a scalar Young absorption returns a
forcing-square envelope with the expected lambda_{s/2,2}^{-1} factor.
Pre-Young Neumann-corrector energy estimate.
The coefficient energy of the centered mean-zero Neumann corrector is bounded by the centered positive-Besov forcing seminorm times the square root of the RHS Poincare radicand for the same corrector gradient.
Young-absorbed Neumann-corrector energy estimate with the centered forcing seminorm kept explicit.
Young-absorbed Neumann-corrector energy estimate with the uncentered forcing seminorm, using the standard invariance of the positive Besov seminorm under subtracting the cube average.
Single-scale force-form consequence of the Young-absorbed Neumann-corrector energy estimate.
This is the local scalar estimate needed before averaging the corrector-energy
component over descendants: the two terms in the Young envelope are both
absorbed into the same s^{-2} lambda^{-1} N^2 [g]^2 scale.